Advanced LIGO Two-Stage Twelve-Axis Vibration Isolation and Positioning Platform. Part 2: Experimental Investigation and Tests Results

This paper presents the results of the past seven years of experimental investigation and testing done on the two-stage twelve-axis vibration isolation platform for Advanced LIGO gravity waves observatories. This five-ton two-and-half-meter wide system supports more than a 1000 kg of very sensitive equipment. It provides positioning capability and seismic isolation in all directions of translation and rotation. To meet the very stringent requirements of Advanced LIGO, the system must provide more than three orders of magnitude of isolation over a very large bandwidth. It must bring the motion below 10^(−11) m/√Hz at 1 Hz and 10^(−12) m/√Hz at 10 Hz. A prototype of this system has been built in 2006. It has been extensively tested and analyzed during the following two years. This paper shows how the experimental results obtained with the prototype were used to engineer the final design. It highlights how the engineering solutions implemented not only improved the isolation performance but also greatly simplified the assembly, testing, and commissioning process. During the past two years, five units have been constructed, tested, installed and commissioned at each of the two LIGO observatories. Five other units are being built for an upcoming third observatory. The test results presented show that the system meets the motion requirements, and reach the sensor noise in the control bandwidth.

[1]  G. M. Harry,et al.  Advanced LIGO: the next generation of gravitational wave detectors , 2010 .

[2]  Bernard F. Schutz,et al.  The GEO 600 gravitational wave detector , 2002 .

[3]  R. Bork,et al.  Hydraulic external pre-isolator system for LIGO , 2013, 1309.5685.

[4]  T. Hayler,et al.  Update on quadruple suspension design for Advanced LIGO , 2012 .

[5]  D. B. DeBra,et al.  Review: Requirements for a Ground Rotation Sensor to Improve Advanced LIGO , 2009 .

[6]  Robin T. Stebbins,et al.  An ultra-low-noise, low-frequency, six degrees of freedom active vibration isolator , 1997 .

[7]  Marco Lops,et al.  The VIRGO Project: A wide band antenna for gravitational wave detection , 1990 .

[8]  Kenneth A. Strain,et al.  GEO 600 triple pendulum suspension system: Seismic isolation and control , 2000 .

[9]  Ben Abbott,et al.  Dynamics Enhancements of Advanced LIGO Multi-Stage Active Vibration Isolators and Related Control Performance Improvement , 2012 .

[10]  Joshua R. Smith,et al.  LIGO: the Laser Interferometer Gravitational-Wave Observatory , 1992, Science.

[11]  Dani Atkinson,et al.  Global Feed-Forward Vibration Isolation in a km scale Interferometer , 2012 .

[12]  James E. Faller,et al.  Low-frequency active vibration isolation system , 1994, Optics & Photonics.

[13]  Robin T. Stebbins,et al.  Multistage active vibration isolation system , 1998 .

[14]  Improvement of the seismic noise attenuation performance of the Monolithic Geometric Anti-Spring filters for gravitational wave interferometric detectors , 2007 .

[15]  Jonathan P. How,et al.  Seismic isolation for Advanced LIGO , 2002 .

[16]  Kentaro Somiya,et al.  Detector configuration of KAGRA–the Japanese cryogenic gravitational-wave detector , 2011, 1111.7185.

[17]  Jeremy Faludi,et al.  Seismic isolation enhancements for initial and advanced LIGO , 2004 .

[18]  Z.Zhang,et al.  Inertial control of the mirror suspensions of the VIRGO interferometer for gravitational wave detection , 2001, gr-qc/0105110.

[19]  K. Kuroda,et al.  The status of LCGT , 2006 .

[20]  Vincent Loriette,et al.  Status of the Virgo project , 2011 .

[21]  Masaki Ando,et al.  Current status of the TAMA300 gravitational-wave detector , 2005 .

[22]  L. Sievers,et al.  A passive vibration isolation stack for LIGO: Design, modeling, and testing , 1996 .

[23]  Vincent Loriette,et al.  Measurements of Superattenuator seismic isolation by Virgo interferometer , 2010 .

[24]  Helena Armandula,et al.  Seismic isolation and suspension systems for Advanced LIGO , 2004, SPIE Astronomical Telescopes + Instrumentation.

[25]  P. Nelson,et al.  An active vibration isolation system for inertial reference and precision measurement , 1991 .

[26]  Stefan Hild The status of GEO 600 , 2006 .

[27]  Jonathan P. How,et al.  Low-frequency active vibration isolation for advanced LIGO , 2004, SPIE Astronomical Telescopes + Instrumentation.

[28]  Michael Hillard,et al.  Advanced LIGO two-stage twelve-axis vibration isolation and positioning platform. Part 1: Design and production overview , 2014, 1407.6377.